Quakes in solid quark stars


Autoria(s): Zhou, AZ; Xu, RX; Wu, XJ; Wang, N
Data(s)

01/10/2004

Resumo

A starquake mechanism for pulsar glitches is developed in the solid quark star model. It is found that the general glitch natures (i.e., the glitch amplitudes and the time intervals) could be reproduced if solid quark matter, with high baryon density but low temperature, has properties of shear modulus mu(c) = 10(30-34) erg/cm(3) and critical stress sigma(c) = 10(18similar to24) erg/cm(3). The post-glitch behavior may represent a kind of damped oscillations. (C) 2004 Elsevier B.V. All rights reserved.

Identificador

http://119.78.226.72//handle/331011/8015

http://www.irgrid.ac.cn/handle/1471x/82690

Idioma(s)

英语

Fonte

周爱芝;R.X.Xu.Quakes in solid quark stars,Astroparticle Physics,2004,22(0):73

Palavras-Chave #射电天文学 #pulsars #neutron stars #elementary particles
Tipo

期刊论文